We review the main properties, demographics and applications of binary and millisecond
radio pulsars. Our knowledge of these exciting objects has greatly increased in recent years …

The first γ-ray line originating from outside the Solar System that was ever detected is the
511 keV emission from positron annihilation in the Galaxy. Despite 30 years of intense …

ABSTRACT The Fermi Large Area Telescope (LAT) has provided the most detailed view to
date of the emission toward the Galactic center (GC) in high-energy γ-rays. This paper …

Over the last 40 years, an astonishing range of astrophysics has become accessible through
pulsar astronomy. The body of literature on this rapidly growing research area is vast and …

We present precise phase-connected pulse timing solutions for 16 γ-ray-selected pulsars
recently discovered using the Large Area Telescope (LAT) on the Fermi Gamma-ray Space …

We present a new joint analysis of pulsar dispersion measures and diffuse Hα emission in
the Milky Way, which we use to derive the density, pressure and filling factor of the thick disk …

Pulsars are born with subsecond spin periods and slow by electromagnetic braking for
several tens of millions of years, when detectable radiation ceases. A second life can occur …

The dramatic increase in the number of known gamma-ray pulsars since the launch of the
Fermi Gamma-ray Space Telescope (formerly GLAST) offers the first opportunity to study a …

We review the current understanding of the Diffuse Gamma-Ray Background (DGRB). The
DGRB is what remains of the total measured gamma-ray emission after the subtraction of the …

Several groups of authors have analyzed Fermi LAT data in a region around the Galactic
Center finding an unaccounted gamma-ray excess over diffuse backgrounds in the GeV …